activity
20082025
most citedPrecision Measurement of Neutrino Oscillation Parameters with KamLAND

812 citations · 960 across the 8 of their papers we have counts for

collaborators

8 papers

physics.ins-det2025

Background stability and annual modulation test using PICOLON ultra-pure NaI(Tl) detector

PICOLON Collaboration, K. Kotera, D. Chernyak +20

The dark matter observation claimed by the DAMA/LIBRA experiment has been a long-standing puzzle within the particle physics community. NaI(Tl) crystals with radiopurity comparable…

hep-ex2024★ 34 cited

Search for Majorana Neutrinos with the Complete KamLAND-Zen Dataset

S. Abe, T. Araki, K. Chiba +69

We present a search for neutrinoless double-beta () decay of Xe using the full \mbox{KamLAND-Zen 800} dataset with 745\,kg of enriched xenon, corresponding to an expo…

hep-ex2024★ 14 cited

Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande

KamLAND, Super-Kamiokande Collaborations, : +311

Preceding a core-collapse supernova, various processes produce an increasing amount of neutrinos of all flavors characterized by mounting energies from the interior of massive star…

astro-ph.IM2024★ 1 cited

Present status of PICOLON project

K. Fushimi, D. Chernyak, H. Ejiri +24

The existence of cosmic dark matter and neutrino properties are long-standing problems in cosmology and particle physics. These problems have been investigated by using radiation d…

hep-ex2023★ 3 cited

Search for Charged Excited States of Dark Matter with KamLAND-Zen

Zen collaboration, S. Abe, M. Eizuka +64

Particle dark matter could belong to a multiplet that includes an electrically charged state. WIMP dark matter () accompanied by a negatively charged excited state ()…

astro-ph.IM2015★ 30 cited

Dark matter search project PICO-LON

K. Fushimi, H. Ejiri, R. Hazama +12

The PICO-LON project aims at search for cold dark matter by means of highly radio-pure and large volume NaI(Tl) scintillator. The NaI powder was purifed by chemical processing to r…

astro-ph.HE2015★ 66 cited

KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars

K. Asakura, A. Gando, Y. Gando +44

In the late stages of nuclear burning for massive stars ($M>8~M_{\sun}$), the production of neutrino-antineutrino pairs through various processes becomes the dominant stellar cooli…

hep-ex2008★ 812 cited

Precision Measurement of Neutrino Oscillation Parameters with KamLAND

The KamLAND Collaboration

The KamLAND experiment has determined a precise value for the neutrino oscillation parameter and stringent constraints on . The exposure to nuclear reactor an…